Chapter 26 Observational Evidence for the Big Bangphysics.uwyo.edu/~pjohnson/astro1050/Lecture 25...

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________________________________________________________________________ Chapter 26 Observational Evidence for the Big Bang ________________________________________________________________________ Under heaven and Earth there is more than one can imagine. --Shakespeare What is inconceivable about the universe is that it is at all conceivable. --Einstein Chapter Preview Some of the most interesting and fundamental questions in astronomy deal with the Universe as a whole. How big is it? How old is it? How did it originate? How is it evolving? It is mind- boggling that by measuring distances and properties of faraway galaxies we can use this information to build theories of the origin of our Universe, the totality of all matter, radiation, and space that can be probed. What is even more incredible is that these theories are testable. In this chapter, we will examine the Big Bang theory of the Universe, the theory that explains the observed velocity-distance relationship for galaxies as the result of an expanding Universe that formed in a creation event. The Universe was infinitesimally small and infinitely hot immediately after this Big Bang. We can still see the cosmic fireball radiation from this creation event 13 billion years ago. Key Physical Concepts to Understand: General Relativity and cosmology, an expanding Universe, determination of the age of the Universe, the steady state cosmology, cosmic background radiation

Transcript of Chapter 26 Observational Evidence for the Big Bangphysics.uwyo.edu/~pjohnson/astro1050/Lecture 25...

Page 1: Chapter 26 Observational Evidence for the Big Bangphysics.uwyo.edu/~pjohnson/astro1050/Lecture 25 The Big Bang.pdfChapter 26 – Observational Evidence for the Big Bang Under heaven

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Chapter 26 – Observational Evidence for the Big Bang

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Under heaven and Earth there is more than one can imagine.

--Shakespeare

What is inconceivable about the universe is that it is at all conceivable.

--Einstein

Chapter Preview

Some of the most interesting and fundamental questions in astronomy deal with the Universe as

a whole. How big is it? How old is it? How did it originate? How is it evolving? It is mind-

boggling that by measuring distances and properties of faraway galaxies we can use this

information to build theories of the origin of our Universe, the totality of all matter, radiation,

and space that can be probed. What is even more incredible is that these theories are testable. In

this chapter, we will examine the Big Bang theory of the Universe, the theory that explains the

observed velocity-distance relationship for galaxies as the result of an expanding Universe that

formed in a creation event. The Universe was infinitesimally small and infinitely hot

immediately after this Big Bang. We can still see the cosmic fireball radiation from this creation

event 13 billion years ago.

Key Physical Concepts to Understand: General Relativity and cosmology, an expanding

Universe, determination of the age of the Universe, the steady state cosmology, cosmic

background radiation

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Web Videos (Youtube)

Why are we here?

http://www.youtube.com/watch?v=EUe_Vfi5IL0&feature=related

Birth of the Universe

1. http://www.youtube.com/watch?v=NEZWtrvxyow&feature=related

2. http://www.youtube.com/watch?v=7WiBET8H3x0&feature=related

3. http://www.youtube.com/watch?v=uD8uFCQkpDE&feature=related

4. http://www.youtube.com/watch?v=gr8zLAxPs-A&feature=related

5. http://www.youtube.com/watch?v=_l0yxRRCrfk&feature=related

I. Introduction

Never has so much been made from so little. From Slipher’s red shift measurements of forty

galaxies came the Hubble law describing the relationship between galaxy distance and velocity

measurements. From this small amount of data, it was inferred that the Universe has expanded

and continues to expand from the creation event. A model of this Big Bang has led for the first

time to answers to some of the philosophical and previously unanswerable fundamental

questions of the origin and evolution of the Universe: What is the global structure of the

Universe? Is it evolving? Is it finite or infinite?

Newton believed the Universe to be infinite. He understandably looked at the Universe through

the perspective of a scientist primarily concerned with gravity. If the Universe were finite, why

wouldn’t gravity cause it to collapse? He inferred that the matter in the Universe must be

distributed throughout a volume of infinite extent, so that the gravitational pull on any one point

is near zero, or equal in all directions. Gravity does indeed dominate the structure of the

Universe, and his concern with the collapse of the Universe was prophetic.

We know now that the Universe is not only finite in size, but that the light from distant objects is

red shifted. At great distances light from galaxies and the stars contained in them recede at

velocities near the speed of light, reducing their energy, as received by us, considerably. We will

examine the evidence supporting this modern view of the Universe.

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II. General Relativity and Cosmology

Einstein’s theory of General Relativity (Chapter 20) was developed at a time when most

scientists considered the Universe as a whole static, or unchanging. In 1917, Einstein applied his

General Theory of Relativity to the Universe in its entirety, and found that to maintain a static

Universe he needed to add a "cosmological constant", or fudge factor (depending on one’s point

of view), to his equations. In 1919, the Dutch physicist W. de Sitter obtained a solution to

Einstein’s cosmological equations, without a cosmological constant, for the extreme case of a

Universe with no matter. In this solution, any particles introduced into the Universe would move

apart with velocities that would increase with time. In 1922, the Russian mathematician A.

Friedmann obtained the solutions to Einstein’s equations for matter-filled Universes, also

without a cosmological constant. The results were three classes of solutions: open, marginally

bound, and closed Universes. We will assume that in each case the Universe begins as an

expansion from a singularity, which we can think of as a point. The open Universe is

characterized by an unbounded expansion from a point that continues forever (Figures 1). A

closed Universe expands from a singularity, reaches a maximum size, and then collapses into a

singularity again. The marginally bound Universe is at the boundary between an open Universe

and a closed one. In a marginally bound Universe, expansion proceeds from a singularity with

the expansion rate slowing at a decreasing rate, as the Universe forever approaches a fixed size.

Figure 1. The evolution of the size of the Universe for closed, open, and marginally bound Big

Bang Universes. If the Universe is open, it will increase in size forever. If it is closed, its

expansion velocity is decelerating causing it to eventually reverse its expansion and decrease in

size. An oscillating Universe is a special type of closed Universe that repeats this cycle of

expansion and contraction. In a marginally bound Universe the expansion continues forever but

at an ever-decreasing rate. P 632-33.3.

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III. Galaxy Red Shifts and the Expansion of the Universe

The discovery by Hubble in 1929 that galaxies are moving away from each other with a velocity

proportional to their distance (according to the Hubble law, velocity = H distance, where H is

the Hubble constant) was one of the major scientific discoveries of the 20th

century. The Hubble

law provided hard experimental verification to the Einstein model of the Universe, without the

cosmological constant. Einstein later confessed that the addition of a cosmological constant to

his equations was the biggest mistake of his career. The distance red shift relationship also

confirmed the Friedmann models of the Universe.

Subsequent measurements have shown that all distant galaxies are moving away from us

and that the Hubble law is the same in all directions. Does this mean that all galaxies in the

Universe are expanding with the Milky Way at the center of the expansion? There has been

a historical tendency for humans to regard the Earth as the center of the Universe, or the Sun as

the center of the Milky Way, or now, the Milky Way as the center of the Universe. This

assumption was found in error in the first two cases, and we will soon see it is not true in the

third instance either.

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A. Raisin Bread Model of the Universe - an Ant’s Perspective

To see how an expanding Universe would look from any location therein, we’ll model it in

familiar terms. Imagine the Universe as a loaf of rising raisin bread with raisins dotting the loaf's

interior a uniform spacing (Figure 2). We’ll consider raisins to be galaxy analogs. But wait! On

one raisin is sitting an unsuspecting ant, munching away with little concern. We are that ant.

Assume that the bread is expanding at a uniform rate. Initially the raisins are spaced 1 centimeter

apart. As the bread rises the spacing changes, to 2 cm in 15 minutes, 3 cm in 30 minutes and so

on. If we look at the raisins along one line of sight, we can measure their distance and the rate at

which they recede (Table 26.1). Using the data in Table 26.1, we can plot the velocity vs.

distance for raisins along this same line of sight. The result, shown in Figure 2b, is a Hubble law

for raisin bread (with apologies to Edwin Hubble). Notice that we have assumed nothing about

the position of our raisin in the loaf or the direction of the line of sight. The Hubble law is valid

for any direction in the raisin bread and from the viewpoint of any raisin. It is not correct to infer

from the observations that one is sitting on some central or preferred raisin in the loaf. Our raisin

has no philosophical significance.

Figure 2. Panel A: A raisin bread model of the Universe. In a loaf of rising raisin bread as in a

Big Bang Universe, an ant standing on any raisin would see all the other raisins moving away

such that the farther the distant raisin, the faster the ant sees it move. FMW 515-25.18 Modified.

Panel B: Hubble law for raisins. Original.

Table 26.1: The Raisin Bread Recipe for an Expanding Universe

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Raisin Time = 0 1 hour 2 hours 3 hours 4 hour

#1 position 1 cm 2 cm 3 cm 4 cm 5 cm

velocity 1 cm/hr

#2 position 2 cm 4 cm 6 cm 8 cm 10 cm

velocity 2 cm/hr

#3 position 3 cm 6 cm 9 cm 12 cm 15 cm

velocity 3 cm/hr

B. The Improved Balloon Model of the Universe – a Finite but Unbounded Universe

The curvature of space-time may produce a finite but unbounded expanding Universe that cannot

be adequately illustrated with the raisin bread analogy. We will upgrade our model to a more

sophisticated balloon model of the Universe to take into account the curvature of space.

As three-dimensional creatures there is no adequate way to visualize the curvature of a three-

dimensional space. It can be conceptually illustrated with the curvature of a two-dimensional

space. Imagine that we live as paper-thin two-dimensional creatures that work and live in a two-

dimensional surface, able to think in terms of North and South but unable to conceive of up or

down. On a local scale our Universe seems flat and extends without limit in all directions. On a

global scale the Universe is spherical and can be modeled as the surface of a balloon. Our

Universe is also an expanding one, the sphere, or balloon surface, growing in diameter at a

constant rate as it is blown up (Figure 3).

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Figure 3. Panel A: A balloon model of the Universe. A two-dimensional creature living on the

surface of a balloon lives in a finite but unbound expanding Universe, just as we live in a three-

dimensional finite but unbound expanding Universe. The balloon creature could set out in one

direction and eventually return to where it started, due to the curvature of the space in which the

creature lives. FMW 565-28.6 Modified. Panel B: Hubble law for dots on a balloon. Original.

To us the inside and outside of our spherical surface have no significance. As we begin to

explore our Universe we can leave our residences and walk in a straight line, eventually to return

to the exact spot from which we started. This occurs because we live in a curved space,

unbounded but of finite extent.

As the balloon expands, we can measure the distances and velocities between points on the

surface of a balloon as we could in the rising raisin bread. The velocities correspond to the

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cosmological red shifts that we see in the real Universe. The results are the same as those in

Table 26.1 and result in a Hubble law for an expanding two-dimensional space (Figure 3).

In the expanding balloon model, we can calculate the scale of the Universe in past epochs. By

extrapolating back in time we find that there was a time when the balloon's radius was zero. We

can say that the observable Universe was a singularity; it had no size.

The same train of reasoning used in the balloon model can be performed theoretically on our

own Universe. We are three-dimensional creatures living in a curved three-dimensional space,

which we can ill-conceive. Our space is finite but unbounded as in the balloon example. That

means we can find no edge and no center to our Universe. Although we could theoretically travel

in a straight line and return to the beginning of our journey, the Universe is far too big to attempt

this experiment, even if we could travel at the speed of light. Extrapolating back in time there

was an instant in the past when the size of the observable Universe was zero. Whatever happened

before this time has no scientific meaning as space and time originated at this epoch in the past

and has been expanding since. No measurement allows us to explore times before this event or

outside our observable Universe. The event of the origin of space-time was the violently

energetic event called the Big Bang, before which space and time have no meaning.

We say that the observable Universe had zero size at the time of the Big Bang. Does that

imply that the size of the Universe is and was finite? No, it does not. The physical size of the

Universe may have been infinite but we say that the observed size was zero. Even if the Universe

was infinite in size at the moment of the Big Bang, space and light were created at that instant

and light has only been able to travel distances of ct, where c is the speed of light and t the age of

the Universe (Figure 3a). The radius of the observable Universe is then ct. If the Universe is 13

billion years old, the size of the observable Universe expanded from zero radius at the Big Bang

to 13 billion light years at the present epoch.

Where did the Big Bang occur? Since space was created in the Big Bang, it didn't occur at a

single location, it occurred everywhere simultaneously. Think of the Big Bang as the sudden

creation of a balloon of finite size. To then ask "Where in space did the Big Bang occur?" is

irrelevant.

If the Universe is infinite in size, how can we quantify its expansion? The Universe can be

parameterized in terms of its scale, which we can think of as the mean distance between galaxies,

R. As the Universe expands, the distance between galaxies becomes larger so R increases. This

increase occurs whether the Universe began as finite or infinite. Although this behavior is

counterintuitive (much about cosmology is impossible to comprehend), the Universe may have

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begun as an expanding infinite Universe that has continuously increased in scale factor from the

Big Bang on.

It should be emphasized that the cosmological velocities of galaxies associated with the

Universal expansion are not ordinary velocities. Galaxies are not moving apart through space,

but are moving with the expansion of space. Each galaxy can be viewed as being at rest with the

space around it, except for small random local velocities, like those resulting from the

gravitational attraction of a galaxy to a nearby galaxy cluster.

If we look at distant galaxies, we view them as they were when the light that we see left those

galaxies on its journey to Earth. A galaxy at a distance of 5 billion light years appears as it did 5

billion years ago. Nonetheless, observers in all galaxies in the Universe can agree on a universal

time scale, e.g., the number of years after the Big Bang. Each observer in the Universe would see

a similar local Universe at any given epoch of cosmic universal time, but would view earlier

epochs when looking out at distant galaxies, as a result of the finite velocity of light. Aliens in

other galaxies might now be viewing the Milky Way as a quasar because they are viewing it as it

looked billions of years ago. We can only see distant stars and galaxies as far as the look-back

time corresponding to the age of the Universe.

IV. Age of the Universe

In the 1940s, American Physicist George Gamow proposed that the Universe began in an

explosion, which we now call the Big Bang. When did the Big Bang occur? A simple

calculation gives us an estimate of the length of time that has passed since the creation event. If

we reverse the cosmological expansion by traveling back in time, galaxies were closer in the

past; at times near the time of the Big Bang all matter, all points in the observable Universe, were

in the same infinitesimal neighborhood. The age of the Universe can be calculated by assuming

that the distance between any two points in the expanding Universe is equal to the age of the

expansion times the relative expansion velocity between the two points. We can use the distance

between a distant galaxy and the Milky Way and the velocity that the distant galaxy has been

receding to estimate the age of the Universe:

Equation 26.1: Age of the Universe = galaxy distance/galaxy velocity.

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Rearranging the Hubble law gives us: H = galaxy velocity/galaxy distance.

Combining Equation 26.1 with the Hubble law produces the following:

Equation 26.2: Age of the Universe = 1/H.

With the currently accepted Hubble constant of 75 km/s/megaparsec, we compute an age of 13

billion years. The actual age of the Universe may be a few billion years younger or older. It is

comforting that this age is longer than the accepted age of the Solar System and the modeled

ages of the oldest stars in the Milky Way. If it were otherwise there would be a contradiction.

This satisfactory state of affairs was not always so. In 1997, estimates of the age of the Universe

were actually less than estimates of the ages of globular clusters, 16-18 billion years. New stellar

measurements caused astronomers to revise the ages of globular clusters to anywhere from 9 to

15 billion years old.

Math box: Let’s estimate the age of the Universe from H.

If the age of the Universe is 1/H and H = 75 km/s/megaparsec, then we can determine the age by

the following:

1 megaparsec = 3 1019

km, so

age of the Universe = 1/H = 1 / 75 km/s/ 3 1019

km = 4 1017

seconds

There are 3 107 seconds in one year, so the age of the Universe is:

4 1017

seconds / 3 107 seconds/year = 13 billion years.

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The calculation above is only an estimate. It assumes a Universe containing no matter. The

gravitational pull among all matter in the Universe gradually slows the universal expansion.

Therefore we should expect that the Universe was expanding more rapidly in the past; galaxies

have separated to greater distances than their current cosmological red shifts would indicate. The

actual age of the Universe may be somewhat less than 13 billion years, depending on the mean

density of matter in the Universe.

As we look further and further out in the Universe, we are looking back in time. If the Universe

is 13 billion years old, we shouldn’t be able to see any objects more than 13 billion light years

distant. At a distance of a little less than 13 billion light years, we might actually be able to see

galaxies being formed.

V. A Rival Model: the Steady State Cosmology

Hubble’s original measurements gave an H of 550 km/s/megaparsec, ten times the current

estimate, giving an age of the Universe of 2 billion years, compared to the estimated 4.6 billion

year age of the Earth. This was a result of errors in distance calibration, which have improved

since. This enormous discrepancy between the age of the Earth and the age of the Universe

spurred a flurry of theoretical activity. In 1948, Fred Hoyle, Herman Bondi, and Thomas Gold

proposed a model of the Universe called the Steady State Theory in which the Universe was

assumed homogeneous, isotropic (appearing the same in all directions), and infinite and

unchanging in space and time. The latter is unique to the Steady State Theory. Galaxies would

recede from each other with apparent velocities in proportion to their distance, obeying Hubble’s

law. Essentially, the Steady State Universe is an infinite Universe that expands. Ordinarily this

expansion would cause a decreasing mean density of matter. In order to maintain an unchanging

Universe, the density of matter should be constant. Hoyle, Bondi, and Gold proposed that matter

must be created continuously throughout the Universe to maintain a constant density (Figure 4).

Although this theory seems unsettling, it can be argued that it is no more difficult to accept than

the sudden creation of the Universe in the Big Bang. The direct creation of matter in the Steady

State Theory only amounted to about 1 atom per cubic meter every billion years or so, so that it

would be undetectable. The heated debate between the Big Bang and Steady State theories lasted

until 1964 and the discovery of the cosmic background radiation, light from the Big Bang.

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VI. Independent Confirmation of the Big Bang: Cosmic Background Radiation

After World War II, physicist George Gamow, of George Washington University, proposed that

the Universe immediately after the Big Bang was incredibly hot, filled with high intensity high-

energy photons called the cosmic background radiation. Physicists Ralph Alpher and Robert

Herman of Johns Hopkins proposed shortly thereafter that as the universe expanded the cosmic

background radiation cooled and was red shifted (Figure 5).

Figure 4. Drawing of look-back time and galaxy evolution. Original.

Figure 5. The Steady State cosmology and the creation of matter. This highly exaggerated

schematic shows that as the Universe expands, some galaxies leave the dashed box representing

a fixed volume, but new matter (galaxies) is created to maintain a constant mass density within

the box. P 607-33.10 Modified.

Figure 6. Blackbodies at various red shifts corresponding to cosmic background radiation at

different times after the Big Bang. Modify. Chaisson.

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In 1964, Arno Penzias and Robert Wilson, Bell Telephone Laboratory physicists, built a

microwave antenna to relay phone calls from Earth-orbiting satellites. With it, they detected a

signal emanating from the sky in all directions. They initially believed this to be a problem with

their instrument. In 1965, after laboriously trying to eliminate this apparently spurious signal

from their antenna, they concluded that it was a nearly uniform emission from the sky. This

microwave radiation was the cosmic background radiation predicted by Gamow, Alpher, and

Herman. Penzias and Wilson are credited with the first detection of the cosmic background

radiation and for this discovery, they won the 1978 Nobel Prize in physics. This detection of

cosmic fireball radiation was the first experimental verification of the Big Bang

independent of the velocity red shift relation.

More recent and precise measurements of the cosmic background show that it has a blackbody

spectrum with a temperature of 2.73 degrees (Figure 6). It is commonly referred to as the 3-

degree background radiation.

After the Big Bang, the matter and radiation in the Universe cooled as the Universe expanded.

Gamow, Alpher and Herman predicted that about 700,000 years after the Big Bang the Universe

would cool to about 3,000 K, cool enough for electrons to combine with individual protons,

forming hydrogen atoms. Individual charged electrons and protons are relatively opaque to

electromagnetic radiation. When electrons and protons combine to form uncharged hydrogen

atoms, they become quite transparent to most electromagnetic radiation. When the Universe was

opaque, in the first 700,000 years after the Big Bang, frequent interactions between light and

matter, in which photons scattered off of electrons and protons, bound matter and radiation to the

same volume of space. As matter cooled and formed, uncharged hydrogen atoms, light, and

matter were free to go their own ways; matter, no longer pushed around by light as in some

cosmic blender, was free to collapse into mass condensations, including protogalaxies. When

light and matter decoupled, theory predicts that radiation would have had a blackbody spectrum

of 3,000 – 4,000 K.

The cosmic background radiation filled all of space. When we observe the cosmic background

radiation today, we are looking at radiation coming from a distance corresponding to the look-

back time of the age of the Universe minus 700,000 years, just as when we look at a galaxy at a

distance of 5 billion light years we are looking back 5 billion years in time. The main difference

is that a galaxy is seen only in one direction in space, while the cosmic background radiation

comes from all directions because it fills space. The 3,000 K background radiation should

experience the same kind of cosmological red shift that galaxies do. The radiation we observe

700,000 years after Big Bang would be red shifted by a factor of roughly 1,000, from the visible

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to a wavelength of about a millimeter (corresponding to temperatures of 3,000 K to nearly 3 K).

This is the same millimeter-wavelength radiation detected by Penzias and Wilson.

The Cosmic Background Explorer satellite, COBE, was launched in 1989 to map the cosmic

background radiation (Figure 7). COBE has shown that the cosmic background is isotropic on a

large scale to one part in 1000, with the exception of an additional red shift in one direction due

to the combined velocity of the Earth about the Sun, the Sun about the center of the Milky Way,

and the Milky Way through the Universe. The entire Milky Way appears to be moving 600 km/s

relative to the neighboring Universe as the Milky Way and Local Group appear to be pulled

toward four nearby galaxy clusters and a massive supercluster. COBE measured slight

differences in the intensity of the cosmic background radiation that may indicate clumps of

matter 500 million light years across from which galaxies and galaxy clusters formed (Figure 8).

Figure 7. Panel A: A COBE (Cosmic Background Explorer) cosmic background spectrum

compared to a 2.73 K blackbody. FMW 575-28.15 or P 612-33.16. Panel B: The COBE

satellite. P 612-33.15.

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Figure 8. A COBE map of the Universe showing the anisotropy of the cosmic background

temperature. Black represents the coolest temperatures, red the hottest. FMW chapter cover or

APOD, NASA.

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In the next chapter, we will see additional support of the Big Bang; the abundances of lithium

and helium in the oldest stars in the Universe agree with the predictions of the Big Bang theory

for elemental abundances in the early Universe.

Summary

The Theory of General Relativity was developed by Einstein in 1917 and used by de Sitter in

1919 and Friedmann in 1922 to show that the natural state of the Universe is one of the

expansion of space. Hubble confirmed this in 1929 with his discovery that galaxies are moving

away from each other with a velocity proporational to their distance. The age of the Universe can

be calculated by assuming that the distance between any two points in the expanding Universe is

equal to the age of the expansion times the relative expansion velocity between the two points.

The current estimated age of the Universe is roughly13 billion years.

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In 1948, Hoyle, Bondi, and Gold proposed the Steady State Cosmology in which the Universe

was assumed infinite and expanding, obeying the Hubble law. To maintain a constant mean

density of the Universe the continuous creation of matter was required.

Supporting proof of the Big Bang Cosmology came with the discovery of the cosmic background

radiation, radiation with a 2.73 K blackbody spectrum that fills all of space. This fossil radiation

from the Big Bang was predicted by the model of Gamow, Alpher, and Herman, which assumed

an initial Universe that was infinitely hot and infinitesimally small at the moment of creation.

Key Words & Phrases

1. cosmological constant – the constant added to Einstein’s General Theory of Relativity to

keep the Universe from expanding.

2. Steady State Theory - a model of the Universe in which the Universe is assumed to be

homogeneous, isotropic, infinite, and unchanging. To account for the cosmological

expansion matter must be created continuously.

3. three-degree background radiation – cosmic fireball radiation from the Big Bang that

has been red shifted so that it is observed with an intensity distribution vs. wavelength

like a 2.73-degree blackbody.

Review for Understanding

1. Why do astronomers believe that the Universe is expanding?

2. What is the difference between 1/H and the actual age of the Universe (from the moment

of the Big Bang)? Which is greater?

3. List observational evidence in favor of and against each of the following: (a) the Big

Bang Theory, and (b) the Steady State Theory.

4. What is the Steady State Cosmology?

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5. How can the Universe not have a center?

6. What is the cosmic background radiation and how did it originate?

7. Why is a low temperature, 2.7 K, measured for the cosmic background radiation when it

had an extremely high temperature immediately after the Big Bang?

8. Why do astronomers believe that the Universe was extremely hot and dense immediately

after the Big Bang?

Essay Questions

1. If you were located in a galaxy near the boundary of our observable Universe, would the

galaxies in the direction of the Milky Way appear to be approaching or receding from

you? Explain.

2. What was the scientific importance of the discovery of the cosmic background radiation?

3. Why should we as a society be interested in funding cosmological research with tax

dollars?